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Multi-Fibers Bundles As a New Model for High-Dimensional Spacetimes

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Multi-Fibers Bundles As a New Model for High-Dimensional Spacetimes Multi-Fibers Bundles as a new model for high-dimensional Spacetimes. Stephane Collion and Michel Vaugon. Institut de Mathématiques, Université Paris VI, Equipe Géométrie et Dynamique, email: [email protected], [email protected] August 2017 Abstract Around 1920, Kaluza and Klein had the idea to add a fifth dimension to the classical 4-dimensional spacetime of general relativity to create a geometric theory of gravitation and electromagnetism. Today, theoretical evidences, like string theory, suggest the need for a spacetime with more than five dimensions. The mathematical translation of the heuristic idea of a 4-dimensional classical spacetime equipped with extra "small" dimensions, is a fiber bundle structure π : M → M on a (4 + k)- dimensional manifold M , with fiber a compact manifold F of dimension k, more shortly a F -fibration. Kaluza and Klein used a fibration with fiber the standard circle S1, this fiber carrying the electromagnetic potential. Inclusion of other physical interaction would therefore require a F -fibration with F of the form F = S1 ×W , W being a compact manifold. However, with such a F -fibration, they is no naturally defined fiber diffeomorphic to S1 at each point of the manifold, and therefore one looses the possibility to define simply the electromagnetic potential. We want to present in this paper a mathematical structure generalizing the fiber bundle, that enable the possible definition of multiple naturally defined fibers at each point of the manifold, on which therefore one can define objects that depend only on one of the components, S1 or W , of the global (S1 × W ) fiber. Although we do not pretend here to model precisely other known physical inter- actions, we present this geometric structure as a possible way to model or encode arXiv:1709.04171v3 [math.DG] 12 Oct 2017 deviations from standard 4-dimensional General Relativity, or "dark" effects such as dark matter or energy ; (we refer to the authors’ article [3] from which this paper is extracted, but whose purpose is different). Also this geometry was a starting point for the second author’s new approach to a geometric unification of general relativity and quantum physics ( see [19]). 1 1Version 04 10 2017. AMS subject classification: 83C22, 83E05, 83E15 1 Beyond five dimensions, Geometrical setting. 2 In all the paper, (M ,gg) is a semi-Riemannian manifold with metric g, ∇ is its Levi- Civita connection, R and Ric are the Riemann and Ricci curvatures. TpM is the tangent space of M at p. We note ∇∇· T the divergence of a tensor T . In all the paper, we identify, without any comments, a (0, 2)-tensor T with the (2, 0)-tensor T ♯♯ obtained by musical isomorphisms. They represent the same physical object. In particular, the Ein- stein curvature G = Ric − 1/2SS.gg will often be consider as a (2, 0)-tensor, G = Gij. We also consider, for a 2-tensor T , the divergence ∇∇· T as a vector, that is, we identify the 1-form ∇∇· T and (∇∇· T )♯. At last, we shall note eT the endomorphism field g-associated e to T : ∀(uu,vv) ∈ Tp(M ) × Tp(M ) : g(uu, T (v)) = T (uu,vv). 1 Beyond five dimensions, Geometrical setting. Theoretical evidences, like string theory, suggest the need for a spacetime with more than five dimensions. We want to present in this paper a mathematical structure generalizing the fiber bundle, that enable the possible inclusion of such other dimensions that might model geometrically multiple physical effects. Note however that we do not pretend here to model precisely such other fields, but that we just want to present a possible mathematical frame. 1.1 Multiple fibers at each point of spacetime. The mathematical translation of the heuristic idea of a 4-dimensional classical spacetime equipped with extra "small" dimensions is a fiber bundle structure π : M → M on a (4+ k)-dimensional manifold M , with fiber a compact manifold F of dimension k, more shortly a F -fibration. Heuristically, M is then the "classical" spacetime when we neglect things that happen in the fibers. As we said in the abstract, Kaluza and Klein used a fibration with fiber the standard circle S1, this fiber carrying the electromagnetic potential. Indeed, suppose now that (M ,gg) is a 5-dimensional Lorentz manifold equipped with a S1-fibration π : M → M over a 4-dimensional Lorentz manifold M . Then the electromagnetic potential can be defined as the unit timelike vector field Y tangent at each point x ∈ M to the fiber 1 −1 1 Sx := π (π(x)) passing through x, once some orientation on S has been defined. Details, as well as a new approach to these ideas can be found in our article [ref :A new approach to Kaluza-Klein theory.] Now if we want to keep the result obtained for electromagnetism while including other possible interactions, the fiber F should be of the form F = S1 × W where W is a compact manifold of dimension m and S1 is the classical circle. However, to keep results obtained for electromagnetism in 5 dimensions, through objects naturally given by the action of S1, one faces a important issue : at each point x ∈ M , such a fiber bundle gives a natural fiber F = S1 × W through x, but it does not give a natural fiber through x isomorphic to S1 only ; there is no natural splitting of the fiber S1 × W at x. Therefore, such a fiber bundle alone will not furnish an electromagnetic potential Y . A very elegant extension of the structure of fiber bundle, giving a way to define any 1.2 Splitting of a product manifold. 3 number of natural fibers at each point x of a manifold M , was originally proposed by Michel Vaugon in [ref]: it is the nice structure of observation atlases. It will be exposed in section [?] below in details, but we give here a new approach, based on the more classical notions of fibrations and submersions. 1.2 Splitting of a product manifold. A natural way to split a fiber F of the form S × W is based on the following nice construction. Let F , S and W be three compact manifolds and let Φ=(h, f): F → S × W be a diffeomorphism, where h and f are the components of Φ. Then h : F → S and f : F → W are submersions. We then define unambiguously, for any x ∈ F , two fibers at x by : −1 Sx := f (f(x)) −1 Wx := h (h(x)) Because S and W are compact, a theorem of Ehresmann states that these submersions are in fact fibrations. Using the diffeomorphism Φ, we can see that h and f are more precisely fibrations with fibers W and S respectively. Indeed, the restrictions h|Sx : Sx → S and f|Wx : Wx → W are diffeomorphisms whose inverse maps are given respectively by : −1 −1 −1 −1 (h|Sx ) (u) = Φ (u, f(x)). (f|Wx ) (v) = Φ (h(x), v). Thus : • h : F → S is a W -fibration. • f : F → W is a S-fibration. Furthermore, we have a natural splitting of the manifold F as a product of two fibers at a given point : for a given point p ∈ F , we have a natural diffeomorphism: ψp : F −→ Sp × Wp y 7−→ ( Φ−1(h(y), f(p)) , Φ−1(h(p), f(y))) Indeed, the inverse map is given by : −1 F ψp : Sp × Wp −→ (a, b) 7−→ Φ−1(h(a) , f(b)) To prove this, note first that, for (a, b) ∈ Sp × Wp, by definition of the fibers, f(a)= f(p) and h(b) = h(p). Setting y = Φ−1(h(a), f(b)), by definition of Φ and its components h and f, h(y) = h(a) and f(y) = f(b). Therefore, Φ−1(h(y), f(p)) = Φ−1(h(a), f(a)) = a and Φ−1(h(p), f(y))=Φ−1(h(b), f(b)) = b. 1.3 Multi-fiber bundle. 4 1.3 Multi-fiber bundle. We now apply this construction to define a multi-fiber structure on a manifold M . Let M be a manifold. Let S and W be two compact manifolds, and F := S × W . We say that a manifold M is a multi-fiber bundle with fibers (S, W ), or a (S, W )-fibration, if M is given two smooth maps according to the following diagram M −→Φ S × W π ↓ M where π : M → M is a F -fibration, and where Φ=(h, f): M → S × W is a map such that, for any p ∈ M , the restriction F ≃ Φ|Fp : p → S × W −1 of Φ to the π-fiber Fp := π (π(p)) is a diffeomorphism. Here again, h and f are the two components of Φ. −1 −1 We shall note x = π(x) for x in M , and Fx := (S × W )x := π (π(x)) := π (x) the π-fiber at a point x of M . (S × W )x is intuitively {x} × F . We also note U := π(U ) for a set U . For a map f : M → N , where N is a manifold, we sometimes note fx the −1 −1 restriction of f to the π-fiber (S × W )x : fx := f|π (x) := f|π (π(x)) := f|Fp . F F ≃ Using now the splitting of each fiber p with the diffeomorphism Φ|Fp : p → S ×W , as seen in the previous section, we can define three natural fibers at each point p ∈ M : For p ∈ M , we define unambiguously three fibers at p : −1 • The global π-fiber Fp := π (π(p)) −1 F • The S-fiber Sp := (f|Fp ) (f(p)), a submanifold of p −1 F • The W -fiber Wp := (h|Fp ) (h(p)), a submanifold of p F where, again, h|Fp and f|Fp are the components of Φ|Fp : p → S × W .
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